lsst.tcc   1.2.2-3-g89ecb63 . ... Classes . Files . ... PVAJT . ... tcc::PVAJT Class Reference . ... PVAJT (double pos , double vel , double accel , double jerk , double t ) . PVAJT (coordConv::PVT const &pvt) . ... extrapolate (double t ) const . ... Definition at line 23 of file pvajt.h . tcc::PVAJT::PVAJT . ... PVAJT tcc::PVAJT::extrapolate . ... double tcc::PVAJT::accel . ... double tcc::PVAJT::jerk . ... double tcc::PVAJT::pos . ... double tcc::PVAJT::t . ... double tcc::PVAJT::vel . ...

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• lsst.coordConv: coordConv::PVT Class Reference
• lsst.tcc: python/tcc/mov/pathSegment.py Source File
• lsst.coordConv: coordConv::Coord Class Reference

... casa::DirectoryIterator . ... Construct the iterator for the working directory. DirectoryIterator (const Directory &dir) . ... DirectoryIterator (const Directory &dir, const Regex &regExpression) . ... Regular expression if given, with this variable it is possible to compare files with regular expression. dirent ** . ... Note that the regular expression is a true regular expression (as defined by class Regex and not a file expression as used in shells. ... File casa::DirectoryIterator::file . ...

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• casacore: casa::MeasComet Class Reference
• casacore: casa::AxesMapping Class Reference
• casacore: casa::TSMShape Class Reference

Stellarium 0.12.3 . ... TextParams Struct Reference . Parameters specifying how to draw text. ... TextParams (const float x, const float y, const QString &string) . Construct TextParams with default parameters. ... TextParams ( Vector3 < F > &position3D, StelProjectorP projector , const QString &string) . Construct TextParams to draw text at a 3D position, using specified projector. ... string   . ... Text string to draw. ... The required string parameter is also set, as is the projector. ...

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• Stellarium: VertexP2 Struct Reference
• Stellarium: StelQGLArrayVertexBufferBackend Class Reference
• Stellarium: VertexP3T2 Struct Reference

Compilation of celestial positions . HyperLeda home | Documentation | Search by name | Search near a position | ... SQL Search | Search the position measurements for an object . B1950 Celestial position . ... precision about 0.1 arcsec . ... 1 arcsec . ... 100 arcsec (1 arcmin) . ... 1000 arcsec (10 arcmin) . ... HyperLeda . ...

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• HyperLEDA documentation: parameter: celpos
• Converting Modules from Apache 1.3 to Apache 2.0 - Apache HTTP Server
• HyperLEDA documentation: compilation of morphology (a102)

... The exact directions of the offsets are parallel to the rows and columns of the CCD on which the aperture is specified. ... It is often useful to explicitly specify the desired rotation of the WFPC2 field-of-view on the sky. ... Figure 7.8 shows the CCD orientation and aperture locations relative to the U3 axis. ... Obtain the Position Angle (PA) of the source axis on the sky, measured in the standard way, North through East. ... desired source angle in field-of-view measured CW from +U3 axis) . ...

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• Apertures
• Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
• Index

Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Developer Documentation . ... This is a first attempt at writing the lessons I learned when trying to convert the mod_mmap_static module to Apache 2.0. ... create per-server config structures */ . ... merge per-server config structures */ . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

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... The spectroscopic model of the source gives , the number of photons received per cm and per second at the earth, from sky position and at energy (differential per solid angle and energy). The number of photons, , detected (per second) in pixel and in PI energy bin centered at is obtained by multiplying by the effective area and applying the response matrix: . ... The correspondence between sky position and detector coordinates depends on the telescope's pointing. ...

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• Command-line position entry.

It seems that every time I try to correct for a pointing error, I have to figure out the sign of the pointing error as reported by the various routines. The pointing error is computed using the heiles calibration scans and by using the turret scans. ... The center of the pattern is the "computed" position of the source using the ra,dec transformation to az,za and any current pointing model. ... X0, Y0 are reported as the error. ... So for turret scans, Add the az,za error to the pointing model. ...

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• byu phased array feed.
• encoderOffsets
• on,off position switching offsets

Full derivation of the projectile motion equations Acceleration is defined as the rate of change of velocity. So, by definition... dv a= dt For the projectile motion case, acceleration is constant. ... To undo differentiation, you need to integrate. ... The right hand is just the integral of the differential of v - i.e. it takes you back to v. For the left hand side, to integrate a constant, multiply it by whatever variable you are integrating against (in this case, t) and add a constant. ...

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... To run the <LAYER> version of the example, select: flower.htm . ... However, if the page had several layers with absolute positions, and you wanted to place another layer in a relative position to one of the existing layers, you could use inline JavaScript to calculate the value for LEFT or TOP . ... In this example, there is really no need to use inline JavaScript to position the last flower layer, since you could just let the TOP value default to its natural value, as in the other flower layers. ...

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• Background color examples
• Index
• Long description for example illustrating positioning with respect to a

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• SADT - Survey Area Definition Tool - for VISTA

Home - News - Download - Documentation - Search - FTP . ... Macros . ... Using these macros also allows a simple find jump history: essentially a position stack is managed (as a string) - the entries (lines) in the string are handled as tag entries. ... The macros use other macro files: . ... Although I have implemented a Return to previous macro, I have not implemented a Goto to next in history list macro, for people who want to go backwards and forwards through their find jump history. ...

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• Dome position

... sin f = y / r . cos f = x / r . ... They are now viewed as new definitions of the sine and cosine, for the polar angle f given by x and y ( a slightly different way of formulating this definition is described further below ). ... sin 2 f + cos 2 f = 1 . ... Angle . ... Many trigonometry texts define the sine and cosine slightly differently, using the so-called unit circle . ... Then the distance AB ("the sine line") equals sin a , and the distance OA ("the cosine line") equals cos a . ...

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• Satellite position in the SE and GSM coordinate systems
• Scientific Programme
• The Favourable Spatial Position

... Positions in 2000 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2001 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2002 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2003 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2004 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . ...

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• Simon Jeffery's Software Store: TAP library
• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |
• Definition of Scientific Misconduct

... Impact on source motion in Galactic coordinate system is given by Kovalevsky (2003), Malkin (2011) l cos b = -A sin l, b = -A cos l sin b, where A = R0 02 /c is the galactocentric acceleration called hereafter the GA constant. ... We just have to return to the traditional many-centuries-old astrometric practice of modelling the position of a celestial object as a linear trend with two parameters: the position at the initial (conventional) epoch and the apparent (proper) motion. ... 2011). ...

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... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...

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• ADASS 2003 Conference Proceedings
• ASC Coordinate Transformation-The Pixlib Library
• The VIMOS Mask Preparation Software

... WSDL for http ://vo.astronet.ru/ws/wcsfix/wcsfix.cgi created by Pod:: WSDL version: 0.05 on Sat Jan 27 20:10:18 2007 -- wsdl :definitions targetNamespace= http ://vo.astronet.ru/wcsFixService xmlns:impl= http ://vo.astronet.ru/wcsFixService xmlns: wsdlsoap = http ://schemas.xmlsoap.org/ wsdl /soap/ xmlns: wsdl = http ://schemas.xmlsoap.org/ wsdl / xmlns:soapenc= ...

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• astro-ph

... Configuration of MIDAS plot # one line per plot defines the box size, position, labelling, date information # P_INDEX : index of plot # XSIZE: size in mm (MIDAS); '-' required # YSIZE: size in mm (MIDAS); '-' required # XOFF: offset from lower left corner, in mm # YOFF: offset from lower left corner, in mm # XLAB: X position of index label (relative to box) # YLAB: Y position of index label (relative to box) # DATE : YES means vertical ...

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• A visual tour
• ESO - Observing conditions: definitions
• ESO - Are there order definition frames with spatial information, i.e. using 9

... Sort a qpoe file using any event attribute. In addition, a filter and a region can be specified. xi> qpsort input qpoe file name: xdata$snr[pi=(1:7)] region descriptor: ``'' # this is the ``null string'' which will cause # entire image to be copied Output qpoe filename: test.qp event definition: medium # possibilities are: peewee, small, medium, large, region type of sort: position # sort the file spatially . ... This is necessary if the qpoe file is to be used with a REGION mask. ...

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• The AstroStat Slog Blog Archive [Jobs] postdoc position at UC Berkeley
• Fixing and Freeing Region Markers
• ChaMP Initial Data Release - X-ray

This WWW form allows the user simplified access to images produced by the NRAO/VLA Sky Survey (NVSS). This service determines which NVSS image is desired based on a celestial position and returns either the image directly or a Web page with a link to the file. ... The NVSS Postage stamp (small FITS file) server can be used to obtain images with other geometries.) ... Web browsers use external viewers to display files like FITS images which they do not understand. ...

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• VLSS Image ftp service Documentation Help for VLSS Image ftp service
• OptInt PmWiki : FDR Todo Lists
• Some notes on the GNU toolchain Bojan Nikolic web pages (r. 329)